Radiation-Absorption, Geometric-Distortion, and Physical-Structure Modeling
| Autor: | D. R. Koehler |
|---|---|
| Rok vydání: | 2017 |
| Předmět: |
010302 applied physics
Physics Nuclear and High Energy Physics media_common.quotation_subject Dark matter Condensed Matter Physics Curvature 01 natural sciences Universe 010305 fluids & plasmas law.invention Computational physics Gravitation law 0103 physical sciences Dark energy Absorption (electromagnetic radiation) Energy source Manifold (fluid mechanics) media_common |
| Zdroj: | IEEE Transactions on Plasma Science. 45:3306-3315 |
| ISSN: | 1939-9375 0093-3813 |
| DOI: | 10.1109/tps.2017.2767295 |
| Popis: | As latter-day experimental interstellar and intergalactic astronomical data are being related to unknown forms of cosmological energies (hypothesized as dark energy and dark matter), we, in the present development, attribute radiation-absorption properties to the universe’s electromagnetic (EM) energy content (plasma energies) or to the universe’s geometric manifold itself. Therefore, for either an EM energy content or a manifold energy content (manifold curvature with radiation absorption), we advance a classical optical attenuation coefficient model to describe energy propagation throughout the universe, thereby providing an alternative analysis and cosmological explanation for the experimental radiative-astronomical data. This modeling is applicable whether one attributes radiation attenuation to the presence of additional universe-bearing EM energy sources or as an interpretation of the geometric manifold as a substantive and locally distortable entity. For the geometric manifold absorption description, the spacetime-absorption-property concept is further utilized to model a radiatively decaying blackbody as the genesis of a propagating decaying shock wave, which in turn is posited as the energy source to mimic a spatially distorted universe. The earlier derived composite coupling constant (gravitational and EM) is inherently incorporated to classify the elements of the seeded universe. Energy densities derived from a distorted-spacetime model are further assimilated in a fundamental manner to describe the ensuing features of the explosive blackbody event. |
| Databáze: | OpenAIRE |
| Externí odkaz: |
|